Method for correcting stray radiation in an x-ray computed tomograph scanner

ABSTRACT

A method for correcting stray radiation for measured values of intensity is proposed that are obtained in an X-ray computer tomography scanner by means of a detector matrix that is situated in a tomography measuring field of the computer tomography scanner and has a multiplicity of detector elements arranged next to one another in a plurality of superimposed detector rows. According to the invention, it is provided in this case that firstly at least one reference distribution of the stray radiation intensity is determined in the row direction of the detector matrix, and that then a stray radiation component of each measured value of intensity is determined starting from this at least one reference distribution, and the measured values of intensity are corrected as a function of their respective stray radiation component. In this case, the stray radiation component of the measured values of intensity of at least a fraction of the detector rows is determined by using a recursion method on the basis of the reference distribution.

[0001] The invention relates to the correction of image artefacts in X-ray computer tomography that are caused by stray radiation.

[0002] Just like beam hardening effects scattering effects can also cause undesired image artefacts in the reconstructed tomographic image of a transradiated layer of a patient or some other object under examination. These image artefacts simulate structures corresponding to no real master of the object under examination, and therefore lead it mistakenly to misinterpretations of the tomographic image. Particularly in the medical sector, such misinterpretations can have grave consequences reaching as far as endangering the life of the patient.

[0003] In order to suppress the stray radiation component in the radiation intensity values measured with the aid of a detector, it is known to collimate on the detector side the X-ray radiation transradiating the object under examination. As a rule, collimators are produced from tungsten, which is very well suited for this because of its high attenuation. However, tungsten has the disadvantage of being very expensive. This cost disadvantage is particularly weighty when use is made as detector of a detector matrix with a multiplicity of detector elements arranged next to one another in a plurality of superimposed detector rows. In the case of such detectors, the depth of the collimator shaft provided for each individual detector element must be enlarged with an increasing number of rows. The outlay on design and materials would be viewed as no longer acceptable starting from a certain number of detector rows.

[0004] It is therefore the object of the invention to render it possible with the aid of a lesser outlay to avoid image artefacts caused by stray radiation in the case of multirow detectors.

[0005] In achieving this object, the invention proceeds according to a first aspect from a method for correcting stray radiation for measured values of radiation intensity that are obtained in an X- ray computer tomography scanner by means of a detector matrix that is situated in a tomography measuring field of the computer tomography scanner and has a multiplicity of detector elements arranged next to one another in a plurality of superimposed detector rows.

[0006] It is provided in this case according to the invention that firstly at least one reference distribution of the stray radiation intensity is determined the row direction of the detector matrix, and that then a stray radiation component of each measured value of intensity is determined starting from this at least one reference distribution, and the measured values of intensity are corrected as a function of their respective stray radiation component, the stray radiation component of the measured values of intensity of at least one fraction of the detector rows being determined by recursion in the following way:

[0007] a) the stray radiation component of the measured values of intensity of a current detector row of the recursion is determined from the measured values of intensity of this current detector row and a primary radiation component of the measured values of intensity of a preceding detector row of the recursion,

[0008] b) the primary radiation component of the measured values of intensity of the preceding detector row is determined from the measured values of intensity of this preceding detector row and the stray radiation component thereof, and

[0009] c) intensity values from the reference distribution of the stray radiation intensity are used as stray radiation component of the measured values of intensity of a first detector row of the recursion.

[0010] If primary radiation is spoken of here, it is understood as that radiation component of the total radiation incident on the detector elements that reaches the detector matrix without being scattered, that is to say on a direct path from the radiation source of the computer tomography scanner. A tomography measuring field is then understood as a measuring zone fitted with detector elements in which the measured total radiation includes a primary radiation component. As a rule, the tomography measuring field is fixed by a diaphragm arrangement on the source side.

[0011] In the solution according to the invention, the stray radiation component is estimated by calculation for all detector rows with the aid of at least one reference distribution. Expensive collimator shafts can thereby be dispensed with. The recursion, which is applied at least for a fraction of the detector rows, offers the basis for taking account of a profile of the stray radiation component that changes across the span of the detector rows.

[0012] In a first refinement of the method according to the invention, the at least one reference distribution of the stray radiation intensity is obtained from measured values of the reference intensity that are obtained by measuring radiation intensity outside the tomography measuring field. The fact that no primary radiation occurs outside the tomography measured field is thereby utilized. Measuring elements arranged there consequently detect only stray radiation. It is easily possible therefrom to determine a distribution of the stray radiation in the row direction, which is then used as reference distribution.

[0013] The radiation intensity will expediently be measured above a first detector row of the detector matrix or/ and below a last detector row of the detector matrix.

[0014] In general, the spatial profile of the stray radiation can be represented by a comparatively low-frequency function. It is therefore sufficient to record measured values for the stray radiation in the row direction only in a relatively coarse array. In other words, the measured values of reference intensity are preferably obtained at measuring points that are situated at a mutual spacing in the row direction of the detector matrix and of which the number is smaller, in particular much smaller than the number of the detector elements per detector row. The reference distribution of the stray radiation intensity can then easily be obtained by interpolation of the measured values of reference intensity.

[0015] It is even possible to obtain one reference distribution by measuring the radiation intensity above the first detector row of the detector matrix, and a further reference distribution by radiation intensity measurement below the last detector row of the detector matrix.

[0016] The recursion should expediently be begun at least in a detector row on the edge of the detector matrix. The assumption that the stray radiation intensity outside the tomography measuring field differs—if at all—only insubstantially from the stray radiation intensity in a detector row at the edge will apply here, as a rule. Consequently, the error that arises when intensity values from the reference distribution are used as stray radiation component of the measured values of intensity from the detector row at the edge will be negligible.

[0017] In the case of a second refinement of the method according to the invention, the at least one reference distribution of the stray radiation intensity is calculated by using the measured values of intensity of at least one detector row of the detector matrix. In particular, it is possible in this case for the reference distribution to be calculated on the basis of a mathematical convolutional model. Such a convolutional model is known, for example, for a computer tomography scanner with detector elements arranged in a single row from B. Ohnesorge: “Untersuchungen der Scatter-Korrektur in Elektronenstrahl-Computertomographen [Research on the scatter correction in electron beam computer tomographs” ] Chair of Information Technology of the University of Erlangen-Nuremberg, Dissertation 1994. By adapting this convolutional model to a multirow detector matrix, it is possible to estimate the stray radiation distribution for a detector row of the matrix by calculation from the measured values of intensity obtained for this detector row.

[0018] It could be objected that the stray radiation distribution could fundamentally be calculated in each case in all detector rows with the aid of the above convolutional model, and that a recursion would then be superfluous. However, convolutional operations can be very demanding computationally. The application of recursion for at least a fraction of the detector rows renders it possible, by contrast, to keep the computational outlay within acceptable limits and, at the same time, to take account of possible changes in the stray radiation distribution from detector row to detector row.

[0019] The reference distribution will expediently be calculated by using the measured values of intensity of a middle detector row of the detector matrix, and the recursion will be begun toward upper and lower detector rows at least in this middle detector row. It goes without saying, however, that the reference distribution can also be calculated with the aid of the measured values of intensity of another detector row, in particular even of a detector row at the edge.

[0020] In order to improve the quality of the results obtained for the stray radiation component of the measured values of intensity, the recursion can be ended after a fraction of detector rows, and a further recursion can be started in a subsequent detector row. The further recursion can be started in this case on the basis of the same or another reference distribution of the stray radiation intensity.

[0021] If the object under examination includes comparatively contrasting structures, the measured values of intensity can change relatively strongly from detector row to detector row or/and within a detector row from detector element to detector element, specifically not on the basis of a rapid change in the stray radiation (which—as already mentioned—changes only comparatively slowly in space, as a rule) but on the basis of spatially changing attenuation properties of the transradiated material. So that such instabilities in the measured total intensity do not substantially falsify the stray radiation components, which are used in the final analysis to correct the measured values of intensity, the stray radiation components determined after carrying out the recursion are preferably subjected to low pass filtering in the column direction and, if desired, also in the row direction of the detector matrix. The low pass filtering filters out from the recursively determined stray radiation components such changes of intensity as have a comparatively high spatial frequency. These are regularly based on changes in the attenuation properties. The filtered stray radiation components thus reproduce the low frequency profile of the stray radiation very well. The measured values of intensity are then corrected as a function of their respective filtered stray radiation component.

[0022] A refinement of the estimate obtained for the stray radiation component of the measured values of intensity is possible when starting from two different reference distributions, two values of the stray radiation component are determined for each measured value of intensity, and the measured values of intensity are corrected in accordance with a respective averaged stray radiation component.

[0023] Independently of the recursive determination of the stray radiation component, the idea of determining the reference distribution by means of measuring the radiation intensity outside the tomography measuring field is also intended to be independently detected within the scope of the invention. According to a second aspect, the invention therefore further provides a method for correcting stray radiation for measured values of radiation intensity that are obtained in an X-ray computer tomography scanner by means of a detector matrix that is situated in a tomography measuring field of the computer tomography scanner and has a multiplicity of detector elements arranged next to one another in a plurality of superimposed detector rows. It is provided in this case according to the invention that firstly at least one reference distribution of the stray radiation intensity in the row direction of the detector matrix is obtained from measured values of reference intensity that are obtained by measuring radiation intensity outside the tomography measuring field, and that a stray radiation component of each measured value of intensity is then determined starting from this at least one reference distribution, and the measured values of intensity are corrected as a function of their respective stray radiation component.

[0024] In order to estimate the stray radiation component of the measured values of intensity, it is also possible here to apply the recursion, explained earlier, with the steps a) to c) . However, it is also conceivable to make use as stray radiation component for each measured value of intensity of an intensity value from the reference distribution of the stray radiation intensity. In this case, the reference distribution is simply taken over directly as stray radiation distribution for each detector row. In cases where the stray radiation intensity actually changes only slightly over the span of the detector matrix, it is possible thereby already to achieve very good results. If, by contrast, marked changes in the stray radiation intensity must be dealt with, preference will be given to the recursive mode of procedure.

[0025] It goes without saying that the method according to the second aspect can be configured by means of further features of the method according to the first aspect.

[0026] Moreover, the subject matter of the invention is an X-ray computer tomography scanner which is designed for carrying out the method according to the first or/and second aspect. In particular, in the case of this computer tomography scanner it is possible to provide an auxiliary detector arrangement, arranged outside the tomography measuring field, for obtaining the measured values of reference intensity. Above a first detector row of the detector matrix or/and below a last detector row of the detector matrix the auxiliary detector arrangement can have a plurality of auxiliary detector elements that are arranged at a mutual spacing in the row direction of the detector matrix and of which each supplies one of the measured values of reference intensity. The number of the auxiliary detector elements in the row direction of the detector matrix is in this case preferably smaller, in particular substantially smaller than the number of the detector elements per detector row.

[0027] The invention is explained in more detail below with the aid of the attached drawings, in which:

[0028]FIG. 1 shows a diagram of an embodiment of a CT scanner according to the invention with a multirow detector matrix, and

[0029]FIG. 2 shows a schematic plan view of the detector matrix when viewing in the direction of the arrow II in FIG. 1.

[0030] The CT scanner shown in the figures comprises an X-ray source 10 and a detector arrangement 12. The X-ray source 10 emits X-ray radiation in the shape of a fan, as indicated at 14. An object under examination 16 arranged in the beam path between the X-ray source 10 and the detector arrangement 12 is penetrated by the X-ray radiation. The detector arrangement 12 detects the X-ray radiation present downstream of the object under examination 16. Specifically, the detector arrangement 12 comprises a detector matrix 18 composed of a multiplicity of detector elements 20 that are distributed over a plurality of superimposed rows and are arranged next to one another in each row in the direction of a fan angle β. Four such detector rows are shown by way of example in FIG. 2; however, it goes without saying that the number of the detector rows can differ therefrom as desired and can be 8, 16 or 24, instead, for example. The size of the beam fan 14 in the direction of the fan angle β can be set by means of a diaphragm arrangement 22 that is arranged between the X-ray source 10 and the object under examination 16. The radiation emitted by the X-ray source 10 is likewise bounded by a comparable diaphragm arrangement (not shown) in the column direction of the detector matrix 18, that is to say in a direction z in FIG. 2. In the region of the detector arrangement 12, the diaphragm arrangement 22 and the z-diaphragm arrangement just addressed define a tomography measuring field within which it is possible to detect the primary radiation that strikes the detector arrangement 12 on a straight path from the X-ray source 10 without being scattered in the object under examination 16. The detector matrix 18 is situated completely within this tomography measuring field. Each position in the direction of the fan angle β at which a detector element 20 is located corresponds to a projection channel.

[0031] Each detector element 20 detects the radiation incident in its zone of space and supplies a corresponding intensity measuring signal I_(G)(n, k) to an electronic evaluation and reconstruction unit 24. Here, the index n stands for the number of the row of the detector matrix 18 in which the relevant detector element 20 is located, while k represents the channel number. The evaluation and reconstruction unit 24 firstly carries out a stray radiation correction on the incoming intensity measuring signals I_(G)(n, k) by subtracting a stray radiation component I_(S)(n, k) from the intensity measuring signals I_(G)(n, k). This leaves a primary radiation component I_(P)(n, k) that is representative of the intensity of the primary radiation incident on the respective detector element 20. The evaluation and reconstruction unit 24 then determines from the intensity values I_(P)(n, k) attenuation values that it uses to reconstruct a tomographic image, displayed on a monitor 26, of the transradiated layer of the object under examination 16. It goes without saying that the CT scanner requires projections from a multiplicity of different directions in order to reconstruct the tomographic image. The X-ray source 10 can be moved for this purpose in the direction of the arrow 28 about the object under examination 16.

[0032] In order to be able to carry out the stray radiation correction, the CT scanner is designed to start by determining a reference distribution of the stray radiation intensity in the row direction. This reference distribution specifies for each channel k a reference value I_(Sref)(k) for the stray radiation intensity. In order to determine the reference distribution, the detector arrangement 12 comprises in addition to the detector matrix 18 a plurality of auxiliary detector elements 30 (see FIG. 2). These are situated outside the tomography measuring field and are therefore not struck by primary radiation but by exclusively by stray radiation. The auxiliary detector elements 30 consequently permit measured information to be obtained on the intensity of the stray radiation. The auxiliary detector elements 30 are also connected to the evaluation and reconstruction unit 24 and supply their measuring signals to the same.

[0033] The auxiliary detector elements 30 are arranged above the uppermost row in the z-direction, or/and below the lowermost row in the z-direction, of the detector matrix 18. Since the spatial distribution of the stray radiation can be described in general by a comparatively low frequency function, a coarse array of the auxiliary detector elements 30 suffices i-n the row direction, and so by comparison with the number of detector elements 20 present per row only a substantially smaller number, for example smaller by an order of magnitude, of auxiliary detector elements 30 is preferably provided in the row direction. The evaluation and reconstruction unit 24 then uses interpolation to determine the reference distribution I_(Sref)(k) supplied by the auxiliary detector elements 30. The auxiliary detector elements 30 are expediently distributed at uniform spacings in the row direction; this is not, however, mandatory. Of course, it is not excluded to provide a number of auxiliary detector elements 30 in the row direction that is equal to the number of the detector elements 20.

[0034] It holds in channel k (k=1, . . . N) for the total intensity I_(G)(n, k) measured in the detector row n (n=1, . . . , L) that:

I _(G)(n, k)=I _(P)(n, k)+I _(S)(n, k)  (1)

[0035] The aim of the stray radiation correction carried out in the evaluation and reconstruction unit 24 is firstly to estimate the stray radiation component I_(S)(n, k) as accurately as possible in order subsequently to have available values for the primary radiation component I_(P)(n, k) that are as accurate as possible and can be fed to the image reconstruction.

[0036] Estimation of the stray radiation begins in the uppermost or the lowermost detector row depending on whether the reference distribution I_(Sref)(k) was obtained from the measuring signals of auxiliary detector elements 30 situated above or below the detector matrix 18. It is assumed below that the operation begins in the uppermost detector row. The channel number is no longer specified explicitly in this case, in order to simplify the notation. The following considerations hold, however, for any desired angular positions in the beam fan, and thus for any desired channel numbers. It then holds for the uppermost detector row that:

I _(G)(1)=I _(P)(1)+I _(S)(1)  (2)

[0037] It is assumed for the purpose of determining the primary radiation intensity I_(P)(1) in the uppermost (first) detector row that I_(Sref) and the stray radiation component I_(S)(l) of the first detector row differ from one another—if at all—only negligibly. The primary radiation intensity I_(P)(1) can therefore be calculated in a simple way as follows:

I _(P)(1)=I _(G)(1)−I _(Sref)  (3)

[0038] The primary radiation intensities in all further detector rows can now be determined similarly by assuming that the primary radiation intensity I_(P)(n−1) of the n−1th detector row corresponds approximately to the primary radiation intensity I_(P)(n) of the nth row. With this assumption, the stray radiation intensity I_(S)(n) in the nth row can be calculated recursively as follows from the actually measured total intensity IG(n) in this row and the primary radiation intensity I(n−1) in the preceding row n−1:

I _(S)(n)=I _(G)(n)−I _(P)(n−1)  (4)

[0039] The primary radiation intensity I_(P)(n) of the nth row can then be estimated in accordance with:

I _(P)(n)=I _(G)(n)−I _(s)(n)  (5)

[0040] The assumption I_(P)(n−1)=I_(P)(n) is justified in general in the case of low-contrast structures. If, however, the object under investigation 16 includes contrasty structures such as bone, for example, significant changes can occur in the measured total intensity between consecutive rows or/and channels. The estimated values I_(S)(n) of the stray radiation intensity are subjected to low pass filtering of selectable length, for example with the aid of a median filter, so that such signal instabilities upon transition from row n−1 to row n in the above recursion are not carried over to the calculation of the stray radiation intensities and therefore falsify the I_(P)(n) values. The low pass filtering removes the instabilities discussed. The filtered I_(S)(n) values then reflect a very good estimate of the actual stray radiation intensity. Subsequently, new I_(P)(n) values that are used for image reconstruction are calculated from the filtered I_(S)(n) values by substitution in the above equation (5).

[0041] The low pass filtering can be carried out as one-dimensional filtering in the z-direction, or else as two-dimensional filtering in the z- and row directions.

[0042] If auxiliary detector elements 30 are provided above and below the detector matrix 18, two reference distributions I_(Sref),1 and I_(Sref),2 can be determined, specifically one (I_(Sref),1) from the measuring signals of the auxiliary detector elements 30 situated above the detector matrix 18, and the other (I_(Sref),2) from the measuring signals of the auxiliary detector elements 30 situated below the detector matrix 18. The above method for recursive estimation of the primary radiation intensities can then be carried out twice, specifically once beginning in the uppermost detector row on the basis of the reference distribution I_(Sref),1, and once beginning in the lowermost detector row on the basis of the reference distribution I_(Sref),2. Thus, two values I_(P),1 and I_(P), 2 of the primary radiation intensity that are subsequently averaged are obtained for each detector element 20. The averaged intensity values are then used for the image reconstruction.

[0043] In some instances, it can already suffice to use the reference distribution I_(Sref) obtained with the aid of the auxiliary detector elements 30 as a model for the stray radiation distribution of all the detector rows of the detector matrix 18. The primary radiation intensities I_(P)(n) can then easily be calculated as follows:

I _(P)(n)=I _(G)(n)−I _(Sref)  (6)

[0044] It is also conceivable not to continue the recursion of all the detector rows, but to truncate it after a fraction of the detector rows, for example, after each second, third or fourth detector row or after half of the detector rows, and then to start a new recursion in a new detector row. In this new detector row, the assumption is made again, in a way similar to equation (3), that the stray radiation distribution of this row corresponds to the reference distribution I_(Sref). It is even possible to conceive of proceeding from a different reference distribution upon restarting the recursion. In the case of the above example with auxiliary detector elements 30 above and below the detector matrix, it could be sensible, for example, to carry out a recursion for the upper half of the detector rows on the basis of the reference distribution I_(Sref),1 and to carry out a recursion on the basis of the reference distribution I_(Sref),2 for the lower half of the detector rows, in particular when the detector matrix 18 has a large number of rows, for example 16, 24 or 32.

[0045] The reference distribution I_(Sref) can also be determined in another way than with the aid of the auxiliary detector elements 30. Thus, for example, it is possible to compute the associated stray radiation distribution I_(S)(n) of a row of the detector matrix 18 from the measured values of intensity I_(G)(n) of said row. This stray radiation distribution I_(S)(n) can then be used as reference distribution I_(Sref) in order to estimate for the remaining rows of the detector matrix 18 the stray radiation component of the measured values of intensity of these rows by means of the above recursion method.

[0046] A convolutional model for a single-row detector system is known from the literature, cited above, of B. Ohnesorge for the purpose of computing a stray radiation distribution from measured values of intensity. This model is based on the idea, in principle, that the functional dependences of the scattering angle on the differential active cross sections and scattering energies of Compton and Raleigh scattering justify the assumption that the scattering contributions in a detector channel k that belongs to a fan angle β_(k) decrease with the angular spacing in the fan (β-β_(k)). (Only simple scattering processes are taken into account in the derivation.) A “spacing function” G(β) that can be used for the description then has a maximum at β=β_(k) and sweeps over the angular range (−β_(max)+β_(k), β_(max)+β_(k)) . A stray radiation distribution I_(SC)(β) dependent on the fan angle β is then yielded as follows:

I _(sc)(β)=C _(m)·ƒ(Δz _(st))·(I _(SC,forw)(β){circle over (x)}G(β))·R(β)  (7)

[0047] Here, C_(M) denotes a machine constant and f(Δz_(s1)) a weighting dependent on layer thickness. I_(SC,forw)(β) is a forward stray radiation intensity, calculated in the model of single scattering, with $\begin{matrix} {I_{{SC},{forw}}\left( {{\beta\beta} = {K_{{SC},{forw}} \cdot {I\left( {\beta \left( {{\cdot \left( {- \ln} \right)}\left( \frac{I\left( {\beta(} \right.}{I_{0}} \right)} \right)} \right.}}} \right.} & (8) \end{matrix}$

[0048] K_(SC,forw) is a proportionality constant, I₀ the intensity of the non-attenuated radiation, and I(β) the radiation intensity measured in the fan angle β of the detector system. The scattering contributions of all the beams in the fan to all the detector elements are taken into account in the convolutional equation (7) by the convolutional core G(β). $\begin{matrix} {{G(\beta)} = \left( {1 + \left( \frac{\beta}{A \cdot {\Delta\beta}} \right)^{2}} \right)^{- k}} & (9) \end{matrix}$

[0049] is usually specified as spacing core. A is parameter with which the width can be controlled. It can be determined empirically from image optimizations or from a comparison of stray radiation distributions calculated in the convolutional model and simulated ones.

[0050] It holds for the function R(β) that:

R(β)=1, if βε[−β_(max), β_(max)]; 0 otherwise  (10)

[0051] Further information on the above convolutional model for single-row detector systems can be taken from the literature of B. Ohnesorge.

[0052] This known model can now be modified within the scope of the invention in order to adapt to multirow or two-dimensional detectors such as shown, for example, in FIG. 2. Equation (7) can easily be expanded because of the rotational symmetry of the differential active cross sections with regard to the fan coordinate β and the row coordinate z_(n) (z_(n)=(L/2−n)Δz; (n=1, . . . L)). (Δz represents the row height) The stray radiation intensity I_(SC)(β, z_(n)) is then given by:

I _(SC)(β,z_(n))=C _(M)·ƒ(Δz _(st))·(I _(SC.forw)(β,z _(n)){circle over (x)}G(β,z _(n)))·R(β,z _(n))  (11)

[0053] In this case, C_(M) and f(Δz_(s1)) have the same meaning as above. I_(SC,forw)(β, z_(n)) is, in turn, the forward scattering radiation intensity calculated in the model of single scattering, with $\begin{matrix} {{I_{{SC},{forw}}\left( {\beta,z_{n}} \right)} = {K_{{SC},{forw}} \cdot {I\left( {\beta,z_{n}} \right)} \cdot \left( {- {\ln \left( \frac{I\left( {\beta,z_{n}} \right)}{I_{0}} \right)}} \right)}} & (12) \end{matrix}$

[0054] I(β, z_(n)) denotes the radiation intensity measured in the fan angle β of the nth detector row. It holds for R(β, z_(n)) that:

R(β,z _(n))=1, if βε[−β_(max), β_(max)] and 1≦n≦L; 0 otherwise  (13)

[0055] The spacing core is now: $\begin{matrix} {{G\left( {\beta,z_{n}} \right)} = \left( {1 + \left( \frac{\beta^{2} + \left( \frac{z_{n}}{R_{fd}} \right)^{2}}{A^{\prime} \cdot {\Delta\beta}} \right)} \right)^{- k}} & (14) \end{matrix}$

[0056] Here, A′ in turn denotes the width parameter, β²+(z_(n)/R_(fd))² measures the distance from the detector origin to the detector element in the fan angle β of the nth detector row, and R_(fd) denotes the spacing between the focus and detector of the CT scanner.

[0057] The stray radiation distribution I_(SC)(β, z_(n)) can be calculated in the previous way for an arbitrary row of the detector matrix 18. It is recommended to calculate it for a middle detector row. The stray radiation distribution thus calculated is then used as reference distribution I_(Sref) for the recursion. The recursion is started in the row from whose measured intensity values the reference distribution was calculated. In the case of a middle detector row, both a recursion to upper detector rows and recursion to lower detector rows are started. If the recursion is interrupted after a fraction of detector rows, a new recursion is begun in a new row, preferably with a new reference distribution that was calculated with the aid of the above convolutional model from the measured values of intensity of this new row. A high quality can be achieved in this way in estimating the accurate stray radiation components. 

1. A method for correcting stray radiation for measured values of radiation intensity (I_(G)(n, k) that are obtained in an X-ray computer tomography scanner by means of a detector matrix (18) that is situated in a tomography measuring field of the computer tomography scanner and has a multiplicity of detector elements (20) arranged next to one another in a plurality of superimposed detector rows, characterized in that firstly at least one reference distribution (I_(Sref)(k)) of the stray radiation intensity is determined in the row direction of the detector matrix (18), and in that then a stray radiation component (I_(S)(n, k)) of each measured value of intensity is determined starting from this at least one reference distribution, and the measured values of intensity are corrected as a function of their respective stray radiation component, the stray radiation component of the measured values of intensity of at least one fraction of the detector rows being determined by recursion in the following way: a) the stray radiation component (I_(S)(n, k)) of the measured values of intensity (I_(G)(n, k)) of a current detector row of the recursion is determined from the measured values of intensity (I_(G)(n, k)) of this current detector row and a primary radiation component (I_(P)(n−1, k)) of the measured values of intensity (I_(G)(n−1, k)) of a preceding detector row of the recursion, b) the primary radiation component (I_(P)(n−1, k)) of the measured values of intensity (I_(P)(n−1, k)) of the preceding detector row is determined from the measured values of intensity (I_(G)(n−1, k)) of this preceding detector row and the stray radiation component (I_(S)(n−1, k) thereof, and c) intensity values from the reference distribution (I_(Sref)(k)) of the stray radiation intensity are used as stray radiation component (I_(S)(1, k)) of the measured values of intensity (I_(G)(1, k)) of a first detector row of the recursion.
 2. The method as claimed in claim 1, characterized in that the at least one reference distribution (I_(Sref)(k)) of the stray radiation intensity is obtained from measured values of the reference intensity that are obtained by measuring radiation intensity outside the tomography measuring field.
 3. The method as claimed in claim 2, characterized in that the radiation intensity is measured above a first detector row of the detector matrix (18) or/and below a last detector row of the detector matrix.
 4. The method as claimed in claim 3, characterized in that the measured values of reference intensity are obtained at measuring points that are situated at a mutual spacing in the row direction of the detector matrix (18) and of which the number is smaller, in particular much smaller than the number of the detector elements (20) per detector row, and in that the reference distribution (I_(Sref)(k)) of the stray radiation intensity is obtained by interpolation of the measured values of reference intensity.
 5. The method as claimed in claim 3 or 4, characterized in that one reference distribution (I_(Sref),1(k)) is obtained by measuring the radiation intensity above the first detector row of the detector matrix (18), and a further reference distribution (I_(S-ref),2(kk)) is obtained by radiation intensity measurement below the last detector row of the detector matrix.
 6. The method as claimed in one of claims 3 to 5, characterized in that the recursion is begun at least in a detector row on the edge of the detector matrix (18).
 7. The method as claimed in claim 1, characterized in that the at least one reference distribution (I_(Sref)(k)) of the stray radiation intensity is calculated by using the measured values (I(β, z_(n)) of intensity of at least one detector row of the detector matrix (18).
 8. The method as claimed in claim 7, characterized in that the reference distribution (I_(Sref)(k)) is calculated on the basis of a mathematical convolutional model.
 9. The method as claimed in claim 7 or 8, characterized in that the reference distribution (I_(Sref)(k)) is calculated by using the measured values (I(β, z_(n)) of intensity of a middle detector row of the detector matrix (18), and in that the recursion is begun toward upper and lower detector rows at least in this middle detector row.
 10. The method as claimed in one of claims 1 to 9, characterized in that the recursion is ended after a fraction of detector rows, and a further recursion is started in a subsequent detector row.
 11. The method as claimed in claim 10, characterized in that the further recursion is started on the basis of the same reference distribution (I_(sref)(k) of the stray radiation intensity.
 12. The method as claimed in claim 10, characterized in that the further recursion is started on the basis of another reference distribution (I_(Sref),1(k), I_(Sref),2(k)) of the stray radiation intensity.
 13. The method as claimed in one of claims 1 to 12, characterized in that the stray radiation components (I_(s)(n, k)) determined after carrying out the recursion are subjected to low pass filtering in the column direction and, if desired, also in the row direction of the detector matrix, and the measured values of intensity (I_(G)(n, k)) are corrected as a function of their respective filtered stray radiation component.
 14. The method as claimed in claim 13, characterized in that a median filter is used for the low pass filtering of the stray radiation components (I_(s)(n, k)).
 15. The method as claimed in one of claims 1 to 14, characterized in that starting from two different reference distributions (I_(Sref),1(k), I_(S-ref),2(k)), two values of the stray radiation component are determined for each measured value of intensity (I_(G) (n, k)), and the measured values of intensity (I_(G)(n, k)) are corrected in accordance with a respective averaged stray radiation component.
 16. A method for correcting stray radiation for measured values of radiation intensity (I_(G)(n, k) that are obtained in an X-ray computer tomography scanner by means of a detector matrix (18) that is situated in a tomography measuring field of the computer tomography scanner and has a multiplicity of detector elements (20) arranged next to one another in a plurality of superimposed detector rows, characterized in that firstly at least one reference distribution (I_(Sref)(k)) of the stray radiation intensity in the row direction of the detector matrix is obtained from measured values of reference intensity that are obtained by measuring radiation intensity outside the tomography measuring field, and in that a stray radiation component (I_(s)(n, k)) of each measured value of intensity is then determined starting from this at least one reference distribution, and the measured values of intensity are corrected as a function of their respective stray radiation component.
 17. The method as claimed in claim 16, characterized in that the stray radiation component (I_(S)(n, k)) of the measured values of intensity (I_(G)(n, k)) of at least a fraction of the detector rows is determined by recursion in the following way: a) the stray radiation component (I_(S)(n, k)) of the measured values of intensity (I_(G)(n, k)) of a current detector row of the recursion is determined from the measured values of intensity (I_(G)(n, k)) of this current detector row and a primary radiation component (I_(P)(n−1, k)) of the measured values of intensity (I_(G)(n−1, k)) of a preceding detector row of the recursion, b) the primary radiation component (I_(P)(n−1, k)) of the measured values of intensity (I_(G)(n−1, k)) of the preceding detector row is determined from the measured values of intensity (I_(G)(n−1, k)) of this preceding detector row and the stray radiation component (I_(S)(n−1, k) thereof, and c) intensity values from the reference distribution (I_(Sref)(k)) of the stray radiation intensity are used as stray radiation component (I_(S)(1, k)) of the measured values of intensity (I_(G) (1, k)) of a first detector row of the recursion.
 18. The method as claimed in claim 16, characterized in that for each measured value (I_(G)(n, k)) of intensity use is made as stray radiation component (I_(S)(n, k)) of an intensity value from the reference distribution (I_(Sref)(k)) of the stray radiation intensity.
 19. The method as claimed in one of claims 16 to 18, characterized by further features of at least one of claims 3 to 6 and 10 to
 15. 20. An X-ray computer tomography scanner that is designed for carrying out the method as claimed in one of claims 1 to 15 or/and the method as claimed in one of claims 16 to
 19. 21. The computer tomography scanner as claimed in claim 20, characterized by an auxiliary detector arrangement (30), arranged outside the tomography measuring field, for obtaining the measured values of reference intensity.
 22. The computer tomography scanner as claimed in claim 21, characterized in that above a first detector row of the detector matrix (18) or/and below a last detector row of the detector matrix the auxiliary detector arrangement (30) has a plurality of auxiliary detector elements (30) that are arranged at a mutual spacing in the row direction of the detector matrix and of which each supplies one of the measured values of reference intensity.
 23. The computer tomography scanner as claimed in claim 22, characterized in that the number of the auxiliary detector elements (30) in the row direction of the detector matrix (18) is smaller, in particular substantially smaller than the number of the detector elements (20) per detector row. 